New classes of black hole spacetimes in 2+1 gravity
arXiv:hep-th/9911069 · doi:10.1016/S0370-2693(00)00191-X
Abstract
The electrogravity transformation is applied to the three-dimensional Einstein field equations to obtain new multi-parameter families of black hole solutions. The Bañados-Teitelboim-Zanelli black hole is shown to be a special case of one of these families. The causal structure, associated matter, as well as the mechanical and thermodynamical properties of some of the solutions are discussed.
arXiv comment8 pages
References in corpus (12)
- The Black Hole in Three Dimensional Space Time
- Quasilocal Energy and Conserved Charges Derived from the Gravitational Action
- Geometry of the 2+1 Black Hole
- Temperature, Energy, and Heat Capacity of Asymptotically Anti-De Sitter Black Holes
- Static Charged Black Holes in Dimensional Dilaton Gravity
- Three Dimensional Black Hole Coupled to the Born-Infeld Electrodynamics
- Large quantum gravity effects: Unexpected limitations of the classical theory
- A spacetime dual to the NUT spacetime
- Exact solutions of Einstein and Einstein-scalar equations in 2 + 1 dimensions
- Behavior of Quasilocal Mass Under Conformal Transformations
- On Electrogravity Duality
- A duality relation for fluid spacetime
Cited by in corpus (8)
- Minimal Geometric Deformation in a cloud of strings
- Greybody factors and quasinormal modes for a nonminimally coupled scalar field in a cloud of strings in (2+1)-dimensional background
- Cloud of strings as source in -dimensional gravity
- Gravoelectric-dual of the Kerr solution
- On Kaluza-Klein spacetime in Einstein-Gauss-Bonnet gravity
- Horizon Mechanics and Asymptotic Symmetries with a Immirzi-like Parameter in 2+1 Dimensions
- Isolated Horizons in 2+1 Gravity
- Global monopoles and scalar fields as the electrogravity dual of Schwarzschild spacetime